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Trans-Planckian Censorship and Inflation in Grand Unified Theories

The recently proposed trans-Planckian censorship conjecture (TCC) amounts to the claim that inflation models with an inflationary energy scale larger than Λinfmax∼109GeV belong to the swampland, i.e., cannot be embedded into a consistent theory of quantum gravity. In this paper, we point out that th...

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Autor principal: Schmitz, Kai
Lenguaje:eng
Publicado: 2019
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.physletb.2020.135317
http://cds.cern.ch/record/2695233
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author Schmitz, Kai
author_facet Schmitz, Kai
author_sort Schmitz, Kai
collection CERN
description The recently proposed trans-Planckian censorship conjecture (TCC) amounts to the claim that inflation models with an inflationary energy scale larger than Λinfmax∼109GeV belong to the swampland, i.e., cannot be embedded into a consistent theory of quantum gravity. In this paper, we point out that this constraint can be readily satisfied in D-term hybrid inflation (DHI), which is a well-motivated inflation scenario in the context of supersymmetric grand unification. In DHI, the amplitude of the primordial scalar power spectrum originates from a Fayet–Iliopoulos term of the order of the unification scale, ξ∼1016GeV . At the same time, the TCC results in an upper bound on the corresponding gauge coupling constant of gmax∼10−14 . We are able to show that this constraint translates into an upper bound on the gravitino mass of m3/2max∼10MeV , which opens the possibility that dark matter is accounted for by thermally produced gravitinos, if the reheating temperature is close to Treh∼100TeV . Interestingly enough, a somewhat similar gravitino mass range has recently been derived in a model that aims at explaining dark energy in terms of axion quintessence and resolving the Hubble tension by means of decaying gravitino dark matter.
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spelling cern-26952332023-10-04T07:34:00Zdoi:10.1016/j.physletb.2020.135317http://cds.cern.ch/record/2695233engSchmitz, KaiTrans-Planckian Censorship and Inflation in Grand Unified Theorieshep-thParticle Physics - Theoryastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyThe recently proposed trans-Planckian censorship conjecture (TCC) amounts to the claim that inflation models with an inflationary energy scale larger than Λinfmax∼109GeV belong to the swampland, i.e., cannot be embedded into a consistent theory of quantum gravity. In this paper, we point out that this constraint can be readily satisfied in D-term hybrid inflation (DHI), which is a well-motivated inflation scenario in the context of supersymmetric grand unification. In DHI, the amplitude of the primordial scalar power spectrum originates from a Fayet–Iliopoulos term of the order of the unification scale, ξ∼1016GeV . At the same time, the TCC results in an upper bound on the corresponding gauge coupling constant of gmax∼10−14 . We are able to show that this constraint translates into an upper bound on the gravitino mass of m3/2max∼10MeV , which opens the possibility that dark matter is accounted for by thermally produced gravitinos, if the reheating temperature is close to Treh∼100TeV . Interestingly enough, a somewhat similar gravitino mass range has recently been derived in a model that aims at explaining dark energy in terms of axion quintessence and resolving the Hubble tension by means of decaying gravitino dark matter.The recently proposed trans-Planckian censorship conjecture (TCC) amounts to the claim that inflation models with an inflationary energy scale larger than $\Lambda {inf}^{max}$ ~ 10$^{9}$ GeV belong to the swampland, $i.e$., cannot be embedded into a consistent theory of quantum gravity. In this paper, we point out that this constraint can be readily satisfied in D-term hybrid inflation (DHI), which is a well-motivated inflation scenario in the context of supersymmetric grand unification. In DHI, the amplitude of the primordial scalar power spectrum originates from a Fayet-Iliopoulos term of the order of the unification scale, $\sqrt{\xi}$ ~ 10$^{16}$ GeV. At the same time, the TCC results in an upper bound on the cor responding gauge coupling constant of $g{max}$ ~ 10$^{-14}$. We are able to show that this constraint translates into an upper bound on the gravitino mass of $m {3/2}^{max}$ ~ 10 MeV, which opens the possibility that dark matter is accounted for by thermally produced gravitinos, if the reheating temperature is close to $T {reh}$ ~ 100 TeV. Interestingly enough, a somewhat similar gravitino mass range has recently been derived in a model that aims at explaining dark energy in terms of axion quintessence and resolving the Hubble tension by means of decaying gravitino dark matter.arXiv:1910.08837CERN-TH-2019-171oai:cds.cern.ch:26952332019-10-19
spellingShingle hep-th
Particle Physics - Theory
astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
Schmitz, Kai
Trans-Planckian Censorship and Inflation in Grand Unified Theories
title Trans-Planckian Censorship and Inflation in Grand Unified Theories
title_full Trans-Planckian Censorship and Inflation in Grand Unified Theories
title_fullStr Trans-Planckian Censorship and Inflation in Grand Unified Theories
title_full_unstemmed Trans-Planckian Censorship and Inflation in Grand Unified Theories
title_short Trans-Planckian Censorship and Inflation in Grand Unified Theories
title_sort trans-planckian censorship and inflation in grand unified theories
topic hep-th
Particle Physics - Theory
astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1016/j.physletb.2020.135317
http://cds.cern.ch/record/2695233
work_keys_str_mv AT schmitzkai transplanckiancensorshipandinflationingrandunifiedtheories